Bodies with space-time orbit by gravitation around their *barycenter*, the center of mass. The word *barycenter* is from the Greek βαρύς, heavy + κέντρον, center. The barycenter is one of the foci of the elliptical orbit of each body.

For the two-body case let *m* and *M* be the two masses, and let *r* and *R* be vectors to *m* and *M* respectively. Then the center of mass or barycenter is

(*mr* + *MR*) / (*m* + *M*).

Define the reduced mass *μ* = *mM*/(*m* + *M*). Then the orbit is as if the orbiting body has reduced mass *μ* and there is a stationary central body with mass equal to the total mass (*m* + *M*). That is, the two bodies mutually orbit the center of mass.

Let’s reconsider the orbit in relation to the vasses, the mass inverses, orbiting by *levitation*. For the two-movement case let *ℓ* and *L* be the two vasses, and let *r* and *R* be vectors from an origin to *ℓ* and *L* respectively. Then the center of vass is

(*ℓr* + *LR*)/(*ℓ* + *L*) = (*Mr* + *mR*) / (*m* + *M*).

Define the reduced vass *Λ* = *ℓL*/(*ℓ* + *L*). Then the orbit is as if the orbiting movement has reduced vass *λ* and there is a stationary central movement with vass equal to the total vass (*ℓ* + *L*). That is, the two movements mutually orbit the center of vass.

The result for vass is the same except that the roles of the movements are reversed. One could call the center of vass the *elaphrocenter* after ελαφρός, light (unheavy) + κέντρον, center.